Kullanıcı:Furkandincer/Negatif Kütle

Vikipedi, özgür ansiklopedi

Genel görelilikte[değiştir | kaynağı değiştir]

Negatif kütle uzayın bazı gözlemciler tarafından kütle yoğunluğunun negatif ölçüldüğü bölgelerini tanımlaması için genelleştirilmiştir. Bu Einstein stres enerji tensör bileşeninin büyüklüğünün kütle yoğunluğundan büyük olduğu uzay bölgeleri nedeniyle gerçekleşebilir. Tüm bunlar Einstein'ın genel görelilik teorisinin diğer değişkenlerini ihlal eder, bununla birlikte pozitif enerji durumu teorinin matematiksel tutarlılığı için gerekli değildir. Pozitif enerji durumunun çeşitli versiyonları, zayıf enerji durumu, baskın enerji durumu vs, Matt Visser tarafından matematiksel detayları açısından tartışılmıştır. [1]

Kütle çekimi eylemsizliğe karşı[değiştir | kaynağı değiştir]

Negatif kütleye ilk gönderme 1700'lerde Filojiston teorisinin incelenmesinde metallerin yükseltgenme sırasında kütle kazanması gözlemi sayesindedir.

Newton kütle çekimi teorisini ilk formüle ettiğinden beri , en azından üç kavramsal olarak ayrılmış nicelik; kütle, eylemsizlik kütlesi, aktif yer çekimi kütlesi (yerçekimi kütlesi yer çekimi alanınını kaynağıdır), pasif yerçekimi kütlesi (yerçekimi alanında oluşan kuvvetten anlaşılan kütle) mevcut. Einstein'ın eşdeğerlik ilkesi eylemsizlik kütlesinin pasif kütle çekimine eşit olması gerektiğini var sayar. Momentumun korunumu kanunu pasif ve aktif kütle çekiminin eşit olmasını gerektirir. Bu güne kadar ki tüm araştırmalar bunları gösterdi. Negatif kütleyi hesaba kattığımızda, bu kavramlardan hangisinin negatif olduğu üzerine düşünmek gerekir. Negatif kütlenin birçok analizinde negatif kütle eşdeğerlik prensibi ve momentumun korunumuna uygulanmaya devam edildiği varsayılır. Bu yüzden tüm kütle formları aynıdır.

In his first prize essay for the 1951 Gravity Research Foundation competition, Joaquin Mazdak Luttinger considered the possibility of negative mass and how it would behave under gravitational and other forces.[2]

In 1957, following Luttinger's idea, Hermann Bondi suggested in a paper in Reviews of Modern Physics that mass might be negative as well as positive.[3] He pointed out that this does not entail a logical contradiction, as long as all three forms of mass are negative, but that the assumption of negative mass involves some counter-intuitive form of motion. For example, an object with negative inertial mass would be expected to accelerate in the opposite direction to that in which it was pushed.

There have been several other analyses of negative mass, for example R.H. Price,[4] however none addressed the question of what kind of energy and momentum would be necessary to describe non-singular negative mass. Indeed, the Schwarzschild solution for negative mass parameter has a naked singularity at a fixed spatial position. The question that immediately comes up is, would it not be possible to smooth out the singularity with some kind of negative mass density. The answer is yes, but not with energy and momentum that satisfies the dominant energy condition. This is because if the energy and momentum satisfies the dominant energy condition within a spacetime that is asymptotically flat, which would be the case of smoothing out the singular negative mass Schwarzschild solution, then it must satisfy the positive energy theorem, i.e. its ADM mass must be positive, which is of course not the case.[5][6] However, it was noticed by Belletête and Paranjape that since the positive energy theorem does not apply to asymptotic de Sitter spacetime, it would actually be possible to smooth out, with energy-momentum that does satisfy the dominant energy condition, the singularity of the corresponding exact solution of negative mass Schwarzschild-de Sitter, which is the singular, exact solution of Einstein's equations with cosmological constant.[7] In a subsequent article, Mbarek and Paranjape showed that it is in fact possible to obtain the required deformation through the introduction of the energy-momentum of a perfect fluid.[8]

Runaway motion[değiştir | kaynağı değiştir]

Although no particles are known to have negative mass, physicists (primarily Hermann Bondi in 1957,[3] William B. Bonnor in 1989,[9] then Robert L. Forward[10]) have been able to describe some of the anticipated properties such particles may have. Assuming that all three concepts of mass are equivalent the gravitational interactions between masses of arbitrary sign can be explored, based on the Einstein field equations:

  • Positive mass attracts both other positive masses and negative masses.
  • Negative mass repels both other negative masses and positive masses.

For two positive masses, nothing changes and there is a gravitational pull on each other causing an attraction. Two negative masses would repel because of their negative inertial masses. For different signs however, there is a push that repels the positive mass from the negative mass, and a pull that attracts the negative mass towards the positive one at the same time.

Hence Bondi pointed out that two objects of equal and opposite mass would produce a constant acceleration of the system towards the positive-mass object,[3] an effect called "runaway motion" by Bonnor who disregarded its physical existence, stating:

Such a couple of objects would accelerate without limit (except relativistic one); however, the total mass, momentum and energy of the system would remain 0.

This behavior is completely inconsistent with a common-sense approach and the expected behaviour of 'normal' matter; but is completely mathematically consistent and introduces no violation of conservation of momentum or energy. If the masses are equal in magnitude but opposite in sign, then the momentum of the system remains zero if they both travel together and accelerate together, no matter what their speed:

And equivalently for the kinetic energy:

Forward extended Bondi's analysis to additional cases, and showed that even if the two masses m(−) and m(+) are not the same, the conservation laws remain unbroken. This is true even when relativistic effects are considered, so long as inertial mass, not rest mass, is equal to gravitational mass.

This behaviour can produce bizarre results: for instance, a gas containing a mixture of positive and negative matter particles will have the positive matter portion increase in temperature without bound. However, the negative matter portion gains negative temperature at the same rate, again balancing out. Geoffrey A. Landis pointed out other implications of Forward's analysis,[11] including noting that although negative mass particles would repel each other gravitationally, the electrostatic force would be attractive for like-charges and repulsive for opposite charges.

Forward used the properties of negative-mass matter to create the concept of diametric drive, a design for spacecraft propulsion using negative mass that requires no energy input and no reaction mass to achieve arbitrarily high acceleration.

Forward also coined a term, "nullification" to describe what happens when ordinary matter and negative matter meet: they are expected to be able to "cancel-out" or "nullify" each other's existence. An interaction between equal quantities of positive mass matter (hence of positive energy ) and negative mass matter (of negative energy ) would release no energy, but because the only configuration of such particles that has zero momentum (both particles moving with the same velocity in the same direction) does not produce a collision, all such interactions would leave a surplus of momentum, which is classically forbidden. So once this runaway phenomenon has been revealed, the scientific community considered negative mass could not exist in the universe.

Arrow of time and space inversion[değiştir | kaynağı değiştir]

In 1970, Jean-Marie Souriau demonstrated, through the complete Poincaré group of dynamic group theory, that reversing the energy of a particle (hence its mass, if the particle has one) is equal to reversing its arrow of time.[12][13]

The universe according to general relativity is a Riemannian manifold associated to a metric tensor solution of Einstein’s field equations. In such a framework, the runaway motion prevents the existence of negative matter.[3][9]

Some bimetric theories of the universe propose that two parallel universes instead of one may exist with an opposite arrow of time, linked together by the Big Bang and interacting only through gravitation.[14][15][16]</nowiki> The universe is then described as a manifold associated to two Riemannian metrics (one with positive mass matter and the other with negative mass matter). According to group theory, the matter of the conjugated metric would appear to the matter of the other metric as having opposite mass and arrow of time (though its proper time would remain positive). The coupled metrics have their own geodesics and are solutions of two coupled field equations:[17][18]

The Newtonian approximation then provides the following interaction laws:

  • Positive mass attracts positive mass.
  • Negative mass attracts negative mass.
  • Positive mass and negative mass repel each other.

Those laws are different to the laws described by Bondi and Bonnor, and solve the runaway paradox. The negative matter of the coupled metric, interacting with the matter of the other metric via gravity, could be an alternative candidate for the explanation of dark matter, dark energy, cosmic inflation and accelerating universe.[17][18]

In Gauss's law for gravity[değiştir | kaynağı değiştir]

In electromagnetism one can derive the energy density of a field from Gauss's law, assuming the curl of the field is 0. Performing the same calculation using Gauss's law for gravity produces a negative energy density for a gravitational field.

Gravitational interaction of antimatter[değiştir | kaynağı değiştir]

The overwhelming consensus among physicists is that antimatter has positive mass and should be affected by gravity just like normal matter. Direct experiments on neutral antihydrogen have not been sensitive enough to detect any difference between the gravitational interaction of antimatter, compared to normal matter.[19]

Bubble chamber experiments provide further evidence that antiparticles have the same inertial mass as their normal counterparts. In these experiments, the chamber is subjected to a constant magnetic field that causes charged particles to travel in helical paths, the radius and direction of which correspond to the ratio of electric charge to inertial mass. Particle–antiparticle pairs are seen to travel in helices with opposite directions but identical radii, implying that the ratios differ only in sign; but this does not indicate whether it is the charge or the inertial mass that is inverted. However, particle–antiparticle pairs are observed to electrically attract one another. This behavior implies that both have positive inertial mass and opposite charges; if the reverse were true, then the particle with positive inertial mass would be repelled from its antiparticle partner.

In quantum mechanics[değiştir | kaynağı değiştir]

In 1928, Paul Dirac's theory of elementary particles, now part of the Standard Model, already included negative solutions.[20] The Standard Model is a generalization of quantum electrodynamics (QED) and negative mass is already built into the theory.

Morris, Thorne and Yurtsever[21] pointed out that the quantum mechanics of the Casimir effect can be used to produce a locally mass-negative region of space–time. In this article, and subsequent work by others, they showed that negative matter could be used to stabilize a wormhole. Cramer et al. argue that such wormholes might have been created in the early universe, stabilized by negative-mass loops of cosmic string.[22] Stephen Hawking has proved that negative energy is a necessary condition for the creation of a closed timelike curve by manipulation of gravitational fields within a finite region of space;[23] this proves, for example, that a finite Tipler cylinder cannot be used as a time machine.

Schrödinger equation[değiştir | kaynağı değiştir]

For energy eigenstates of the Schrödinger equation, the wavefunction is wavelike wherever the particle's energy is greater than the local potential, and exponential-like (evanescent) wherever it is less. Naively, this would imply kinetic energy is negative in evanescent regions (to cancel the local potential). However, kinetic energy is an operator in quantum mechanics, and its expectation value is always positive, summing with the expectation value of the potential energy to yield the energy eigenvalue.

For wavefunctions of particles with zero rest mass (such as photons), this means that any evanescent portions of the wavefunction would be associated with a local negative mass–energy. However, the Schrödinger equation does not apply to massless particles; instead the Klein-Gordon equation is required.

Negative bare mass of the electron[değiştir | kaynağı değiştir]

The mass contributed to the total mass of the electron by the cloud of virtual photons, by Einstein's second law, is positive, so the bare mass of the electron is necessarily less than its observed mass. Since the virtual photons have energies greater than twice the electron mass, so they can make the electron-positron pairs needed for charge renormalization, then the bare mass of the source electron must be negative.[24][25][26]

In Special Relativity[değiştir | kaynağı değiştir]

One can achieve a negative mass independent of negative energy. According to mass energy equivalence, mass is in proportion to energy and the coefficient of proportionality is . Actually, is still equivalent to although the coefficient is another constant[27] such as

.[28] In this case, it is unnecessary to introduce a negative energy because the mass is negative even though the energy is positive. That is to say,

Under the circumstances,

When ,

Therefore,

where is invariant mass and invariant energy equals .

Since ,

The negative momentum is applied to explain negative refraction,inverse Doppler effect and reverse Cherenkov effect observed in a negative index metamaterial.Radiation pressure in the metamaterial is also negative[29] because the force is defined as . Interestingly, negative pressure occurs in dark energy too. Using these above equations, the energy–momentum relation should be

Moreover,the kinetic energy is also negative

,

Actually, the negative kinetic energy exists in some models[30] to describe dark energy (phantom energy) whose pressure is negative. In this way, the negative mass is now associated with negative momentum,

negative pressure and negative kinetic energy.

  • Alcubierre drive
  • Antimatter
  • Dark energy
  • Dark matter
  • Exotic matter
  • Mirror matter
  • Warp-field experiments
  • Woodward effect

References[değiştir | kaynağı değiştir]

External links[değiştir | kaynağı değiştir]

Negatif kütle, teorik fizikte normal kütlenin zıt işaretlisi olan varsayımsal madde kavramıdır, örneğin -2 kg. Bu durum bir ya da daha fazla enerji koşulunu ihlal eder ve negatif kütle için çekimin kuvvet olması gerektiği ve pozitif yönlü ivmeye sahip olması gerektiği anlaşmazlığından kaynaklanan bazı garip özellikler gösterir. Negatif kütle, solucan deliği inşa etme gibi bazı kuramsal teorilerde kullanılır. Egzotik maddeye benzeyen en yakın bilinen örnek Casimir etkisi tarafından üretilen sözde negatif basınç yoğunluğunun alanıdır. Genel izafiyet teorisinin kütle çekimini ve pozitif, negatif enerji yüklerinin hareket yasasını iyi tanımlamasına rağmen negatif kütle dolayısıyla başka temel kuvvetleri içermez. Diğer yandan, standart model, temel parçacıkları ve diğer temel kuvvetleri iyi tanımlamasına ve kütle çekimi kütle merkezini ve eylemsizliği derinlemesine içerse rağmen kütle çekimini içermez. Negatif kütlenin kavramının daha iyi anlaşılabilmesi için kütle çekimini açık bir şekilde ifade eden modelle birlikte diğer temel kuvvetler de gerekebilir.

  1. ^ Visser, M. (1995).
  2. ^ Luttinger, J. M. (1951).
  3. ^ a b c d Bondi, H. (July 1957).
  4. ^ Price, R. M. (1993).
  5. ^ Shoen, R.; Yao, S.-T. (1979).
  6. ^ Witten, Edward (1981).
  7. ^ Belletête, Jonathan; Paranjape, Manu (2013).
  8. ^ Mbarek, Saoussen; Paranjape, Manu (2014).
  9. ^ a b Bonnor, W. B. (1989).
  10. ^ Forward, R. L. (1990).
  11. ^ Landis, G. (1991).
  12. ^ Souriau, J. M. (1970).
  13. ^ Souriau, J. M. (1997).
  14. ^ A.D. Sakharov: "Cosmological model of the Universe with a time vector inversion".
  15. ^ Petit, J. P. (1995).
  16. ^ Barbour, J.; Koslowski, T.; Mercati, F. (2014). "Identification of a Gravitational Arrow of Time". Physical Review Letters. 113 (18). doi:10.1103/PhysRevLett.113.181101. "Identification of a Gravitational Arrow of Time". Physical Review Letters 113 (18). doi:10.1103/PhysRevLett.113.181101. <nowiki>
  17. ^ a b Petit, J. P.; d’Agostini, G. (2014).
  18. ^ a b Petit, J. P.; d'Agostini, G. (2014).
  19. ^ Amole, C.; Charman, M. D.; Amole, M.; Ashkezari, W.; Baquero-Ruiz, E.; Bertsche, A.; Butler, C. L.; Capra, M.; Cesar, S.; Charlton, J.; Eriksson, T.; Fajans, M. C.; Friesen, D. R.; Fujiwara, A.; Gill, J. S.; Gutierrez, W. N.; Hangst, M. E.; Hardy, C. A.; Hayden, S.; Isaac, L.; Jonsell, A.; Kurchaninov, N.; Little, J. T. K.; Madsen, S.; McKenna, S. C.; Menary, P.; Napoli, A.; Nolan, P.; Olin, C. Ø.; Pusa, F. (2013).
  20. ^ Dirac, P. A. M. (1928).
  21. ^ Morris, Michael; Thorne, Kip; Yurtsever, Ulvi (September 1988).
  22. ^ Cramer, John; Forward, Robert; Morris, Michael; Visser, Matt; Benford, Gregory; Landis, Geoffrey (1995).
  23. ^ Hawking, Stephen (2002).
  24. ^ Woodward, J. F. (1993).
  25. ^ Woodward, J. F. (1994).
  26. ^ Woodward, J. F. (2013).
  27. ^ Wang, Z.Y, Wang P.Y, Xu Y.R (2011).
  28. ^ Wang,Z.Y. (2015).
  29. ^ Veselago, V. G. (1968).
  30. ^ Caldwell,R.R. (2002).

See also[değiştir | kaynağı değiştir]

[[Kategori:Egzotik maddeler]] [[Kategori:Kütleçekim]] [[Kategori:Varsayımsal nesneler]] [[Kategori:Kütle]] [[Kategori:Solucan deliği teorisi]]